Substructure of a Kelvin‐Helmholtz Vortex Accompanied by Plasma Transport Under the Northward Interplanetary Magnetic Field
Author:
Affiliation:
1. State Key Laboratory of Space Weather National Space Science Center Chinese Academy of Sciences Beijing China
2. Space Science Laboratory University of California Berkeley CA USA
3. University of Maryland Baltimore County Baltimore MD USA
Funder
National Natural Science Foundation of China
Chinese Academy of Sciences
Publisher
American Geophysical Union (AGU)
Subject
Space and Planetary Science,Geophysics
Link
https://onlinelibrary.wiley.com/doi/pdf/10.1029/2021JA029735
Reference73 articles.
1. The Kelvin–Helmholtz instability under Parker-Spiral Interplanetary Magnetic Field conditions at the magnetospheric flanks
2. The THEMIS Mission
3. The THEMIS Fluxgate Magnetometer
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5. Relativity and the Solar Wind: The Maxwell-Equation Origins of the Solar-Wind Motional Electric Field
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1. Density and Magnetic Field Asymmetric Kelvin‐Helmholtz Instability;Journal of Geophysical Research: Space Physics;2024-03
2. Rayleigh‐Taylor Instability Observed at the Dayside Magnetopause Under Northward Interplanetary Magnetic Field;Journal of Geophysical Research: Space Physics;2023-06-27
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